Astronomy:335 Roberta

From HandWiki
Short description: Large main belt asteroid
335 Roberta
Орбита астероида 335.png
Orbital diagram
Discovery
Discovered byAnton Staus
Discovery date1 September 1892
Designations
(335) Roberta
Named afterCarl Robert Osten-Sacken
1892 C
Minor planet categoryMain belt
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc123.58 yr (45137 d)
|{{{apsis}}}|helion}}2.9014 astronomical unit|AU (434.04 Gm)
|{{{apsis}}}|helion}}2.04926 AU (306.565 Gm)
2.47530 AU (370.300 Gm)
Eccentricity0.17212
Orbital period3.89 yr (1422.5 d)
Average Orbital speed18.93 km/s
Mean anomaly355.460°
Mean motion0° 15m 11.095s / day
Inclination5.1005°
Longitude of ascending node148.454°
140.006°
Earth MOID1.03587 AU (154.964 Gm)
Jupiter MOID2.2733 AU (340.08 Gm)
TJupiter3.456
Physical characteristics
Dimensions89.07±2.0 km[1]
Rotation period12.054 h (0.5023 d)
Geometric albedo0.0580±0.003[1]
0.058[2]
B–V = 0.624
U–B = 0.235
FP (Tholen)
B (SMASS)[1]
Absolute magnitude (H)8.96[1]


Roberta (minor planet designation: 335 Roberta) is a large main belt asteroid. It was discovered on 1 September 1892, by German astronomer Anton Staus at Heidelberg Observatory.[3] Roberta was the 12th asteroid that was discovered using photography, and the only asteroid discovery made by Staus.[4]

Photometric observations of this asteroid from multiple sites during 2007 gave a light curve with a period of 12.054 ± 0.003 hours and a brightness variation of 0.13 ± 0.02 in magnitude. This agrees with a result reported in 1992, but differs from period estimates of 8.03 hours and 4.349 reported in 1987 and 2001, respectively.[5]

Under the SMASS classification taxonomy, this asteroid is listed as a B-type; a group that combines both the Tholen B and F types. The spectrum of this object suggests the presence of magnetite (Fe3O4), which gives it the spectrally-blue coloration that is a characteristic of this SMASS class. The spectrum of this asteroid also displays a band feature near 2.9 μm that indicate the presence of a hydrated mineral. This suggests that the asteroid has undergone significant water-based alteration.[2]

335 Roberta was identified as one of three asteroids that were likely to be a parent body for chondrites along with 449 Hamburga and 304 Olga.[6] All three asteroids were known to have low-albedo (not reflect as much light) and be close to "meteorite producing resonances".[6] Chrondrites are the most common type of meteor found on Earth, accounting for over 80% of all meteors.[7] They are named for the tiny spherical silicate particles that are found inside them (those particles are called chondrules).[7]

References

  1. 1.0 1.1 1.2 1.3 1.4 "335 Roberta", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=335, retrieved 11 May 2016 
  2. 2.0 2.1 Yang, Bin; Jewitt, David (September 2010), "Identification of Magnetite in B-type Asteroids", The Astronomical Journal 140 (3): 692–698, doi:10.1088/0004-6256/140/3/692, Bibcode2010AJ....140..692Y 
  3. "Numbered Minor Planets 1–5000", Discovery Circumstances (IAU Minor Planet center), https://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html, retrieved 7 April 2013. 
  4. Kutter, A. (December 1957). "Nachruf auf Anton Staus (Obituary)" (in de). Mitteilungen der Astronomischen Gesellschaft 9: 5. Bibcode1958MitAG...9....5K. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1958MitAG...9....5K. Retrieved 6 July 2016. 
  5. Warner, Brian D. et al. (December 2007), "Lightcurve Analysis of 335 Roberta", The Minor Planet Bulletin 34 (4): p. 99, Bibcode2007MPBu...34...99W. 
  6. 6.0 6.1 Lunar and planetary science: abstracts of papers submitted to the ... Lunar and Planetary Science Conference, Volume 27, Part 1 - Lunar and Planetary Institute, Jan 1, 1996
  7. 7.0 7.1 "ASU - Chondrites". https://meteorites.asu.edu/meteorites/meteorite-types/stony-meteorites/chondrites. 

External links